Multidimensional cosmological and spherically symmetric solutions with intersecting p-branes

Details Multidimensional cosmological and spherically symmetric solutions with intersecting p-branes Multidimensional cosmological and spherically symmetric solutions with intersecting p-branes

1999-01-02

arxiv.org/abs/gr-qc/9901001v2

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

33 pages, Latex., several typos and paragraphs are eliminated Publ.: Proc. of 2nd Samos meeting (1999), Lect. Notes in Phys.,

Scientific paper

Multidimensional model describing the "cosmological" and/or spherically symmetric configuration with n+1 Einstein spaces in the theory with several scalar fields and forms is considered. When electro-magnetic composite p-brane ansatz is adopted, n "internal" spaces are Ricci-flat, one space M_0 has a non-zero curvature, and all p-branes do not "live" in M_0, a class of exact solutions is obtained if certain block-orthogonality relations on p-brane vectors are imposed. A subclass of spherically-symmetric solutions containing non-extremal p-brane black holes is considered. Post-Newtonian parameters are calculated and some examples are considered.

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